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	Telescope alignment based on the structured lighting of collimated laser beam bundles 会议论文 OAI收割 Montréal, Québec, Canada, 2022-8-29 作者: Li ZY(李正阳); Jiang X(姜鑫); Han ZJ(韩子健); Yuan XY(袁祥岩) \| 收藏 \| 浏览/下载：32/0 \| 提交时间：2023/03/22 telescope aberrations alignment method coordinate distortion laser collimator wave-front reconstruction optical collimator
	Computation of misalignment and primary mirror astigmatism figure error of two-mirror telescopes 期刊论文 OAI收割 Journal of Astronomical Telescopes Instruments and Systems, 2018, 卷号: 4, 期号: 1, 页码: 10 作者: Gu, Z. Y.; Wang, Y.; Ju, G. H.; Yan, C. X. \| 收藏 \| 浏览/下载：152/0 \| 提交时间：2019/09/17 active optics alignment misalignments astigmatic figure error nodal aberration theory two-mirror telescope 5th-order optical aberrations rotational symmetry wave-front systems collimation Engineering Instruments & Instrumentation Optics
	Alignment algorithm for three-mirror anastigmatic telescopes based on nodal aberration theory 期刊论文 OAI收割 Journal of Modern Optics, 2018, 卷号: 65, 期号: 16, 页码: 1910-1919 作者: Xing, Z. C.; Hong, Y. F.; Zhang, X. B.; Zhang, B. \| 收藏 \| 浏览/下载：18/0 \| 提交时间：2019/09/17 Aberration theory alignments telescopes active optics 5th-order optical aberrations rotational symmetry wave-front systems Optics
	Training to improve contrast sensitivity in amblyopia: correction of high-order aberrations 期刊论文 OAI收割 SCIENTIFIC REPORTS, 2016, 卷号: 6 作者: Liao, Meng; Zhao, Haoxing; Liu, Longqian; Li, Qian; Dai, Yun \| 收藏 \| 浏览/下载：25/0 \| 提交时间：2018/06/14 Wave-front Aberrations Anisometropic Amblyopia Juvenile Amblyopia Visual Performance Adaptive Optics Adult Amblyopia Defined Letters Vision Eyes Acuity
	A new method for comparing Zernike circular polynomials with Zernike annular polynomials in annular pupils (EI CONFERENCE) 会议论文 OAI收割 2010 International Conference on Computer, Mechatronics, Control and Electronic Engineering, CMCE 2010, August 24, 2010 - August 26, 2010, Changchun, China Jing S.; Dongmei M. 收藏 \| 浏览/下载：25/0 \| 提交时间：2013/03/25 To compare the difference between Zernike annular polynomial and Zernike circular polynomial an approximate mathematic relationship between Zernike annular polynomial coefficients and SEIDEL coefficients is proposed. A new method is applied in comparing experiment. For real interferometric data of annular wave front the SEIDEL aberration calculated in different ways is removed from the original wave front. Residual astigmatism aberration in annular polynomial way is close to zero but defocus and sphere aberration are 0.002709 -0.00182. The residual SEIDEL using annular polynomial is least. Data used in comparison shows that Zernike annular polynomial is more accurate and meaningful for the decomposition of aberrations and the calculation of Seidel aberrations in annular pupil. The calculation in astigmatism aberration is most accurate and those in defocus and sphere aberration are least accurate when the first 9 terms are used in approximate solving SEIDEL. More coefficients are needed to obtain the real SEIDEL. 2010 IEEE.
	Design and tolerance analysis of compensator for high order aspheric surface testing (EI CONFERENCE) 会议论文 OAI收割 2009 International Conference on Optical Instruments and Technology - Optoelectronic Measurement Technology and Systems, October 19, 2009 - October 22, 2009, Shanghai, China 作者: Chen X.; Liu W.; Chen X.; Chen X. 收藏 \| 浏览/下载：29/0 \| 提交时间：2013/03/25 High accuracy is required in surface testing of 90nm nodal point lithography projecting lens. By comparing various aspheric surface testing methods the structure layout of the compensator is a meniscus positive lens combined with a Plano-convex positive lens. The design results indicate that: primary and high order aberrations are balanced well we adopt Offner null compensator to test the aspheric surface in the point diffraction interferometer at last. In this paper MTF exceeds diffraction limit an Offner compensator is presented on the base of the third order aberration theory to test concave aspheric surface root-mean-square (RMS) of wave front error /167. The F-number of the system can achieve F/1.64. By the analysis of the process of aspheric surface testing with the designed system the optical construction parameters of which is determined by introducing equal-quantities spherical aberration to compensate all orders of aspheric coefficients. The field of view of the system is 0.02 a loosen distribution of the tolerance was presented based on the accuracy of measuring apparatus. 2009 SPIE.